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Magnetar spin-down glitch clearing the way for FRB-like bursts and a pulsed radio episode
DOI: 10.1038/s41550-022-01865-y Bibcode: 2023NatAs...7..339Y

Lin, L.; Kouveliotou, C.; Baring, M. G. +16 more

Magnetars are a special subset of the isolated neutron star family, with X-ray and radio emission mainly powered by the decay of their immense magnetic fields. Many attributes of magnetars remain poorly understood: spin-down glitches or the sudden reductions in the star's angular momentum, radio bursts reminiscent of extragalactic fast radio burst…

2023 Nature Astronomy
XMM-Newton 43
A 5.3-min-period pulsing white dwarf in a binary detected from radio to X-rays
DOI: 10.1038/s41550-023-01995-x Bibcode: 2023NatAs...7..931P

Kepler, S. O.; Heywood, I.; Dhillon, V. S. +19 more

White dwarf stars are the most common stellar fossils. When in binaries, they make up the dominant form of compact object binary within the Galaxy and can offer insight into different aspects of binary formation and evolution. One of the most remarkable white dwarf binary systems identified to date is AR Scorpii (AR Sco). AR Sco is composed of an …

2023 Nature Astronomy
Gaia XMM-Newton 33
Vertical wind structure in an X-ray binary revealed by a precessing accretion disk
DOI: 10.1038/s41550-023-01929-7 Bibcode: 2023NatAs...7..715K

Fabian, A. C.; Reynolds, C. S.; Pinto, C. +11 more

The accretion of matter onto black holes and neutron stars often leads to the launching of outflows that can greatly affect the environments surrounding the compact object. An important means of studying these winds is through X-ray absorption line spectroscopy, which allows us to probe their properties along a single sightline, but usually provid…

2023 Nature Astronomy
XMM-Newton 8